NSTX Supported by Electron gyro-scale fluctuations in NSTX plasmas College W&M Colorado Sch Mines Columbia U Comp-X General Atomics INEL Johns Hopkins U LANL LLNL Lodestar MIT Nova Photonics New York U Old Dominion U ORNL PPPL PSI Princeton U Purdue U SNL Think Tank, Inc. UC Davis UC Irvine UCLA UCSD U Colorado U Maryland U Rochester U Washington U Wisconsin David Smith, PPPL with E. Mazzucato 1, W. Lee 2, H. K. Park 2, C. W. Domier 3, N. C. Luhmann, Jr. 3, and the NSTX Research Team 1 PPPL, 2 POSTECH, 3 UC-Davis 50 th Annual Meeting of the Division of Plasma Physics Dallas, TX November 17 21, 2008 Culham Sci Ctr U St. Andrews York U Chubu U Fukui U Hiroshima U Hyogo U Kyoto U Kyushu U Kyushu Tokai U NIFS Niigata U U Tokyo JAEA Hebrew U Ioffe Inst RRC Kurchatov Inst TRINITI KBSI KAIST POSTECH ASIPP ENEA, Frascati CEA, Cadarache IPP, Jülich IPP, Garching ASCR, Czech Rep U Quebec
NSTX is well-suited to investigate the connection between ETG turbulence and electron thermal transport Electron thermal transport anomalous in all confinement regimes in all machines Electron temperature gradient (ETG) turbulence NL GK simulations predict experimentallyrelevant electron thermal transport for ŝ > 0.4 (Nevins et al, PoP 2006) Electron gyro-scale fluctuations k^ρ e d 1 Turbulence & transport in NSTX Large E B flow shear with NBI inferred ITG/TEM suppression ion thermal transport is near neoclassical in H-mode (Kaye et al, NF, 2007 & PRL, 2007) Electron thermal transport remains anomalous what is the mechanism? ETG can be linearly unstable with growth rates exceeding E B flow shear rates NSTX 50 th Annual Meeting of the Division of Plasma Physics November 17 21, 2008 2
Electron gyro-scale fluctuations in NSTX plasmas The NSTX collective scattering system Electron gyro-scale fluctuation measurements and analysis ETG linear critical gradient High-Te L-mode w/ RF heating Core measurements in H-mode w/ NBI heating ETG linear growth rate and EμB flow shear rate Mid-radius measurements in H-mode w/ NBI heating Fluctuation amplitude dependence on B T Fluctuation k-spectra and comparison with GTS simulation Summary NSTX 50 th Annual Meeting of the Division of Plasma Physics November 17 21, 2008 3
Collective scattering encodes the fluctuation k-spectrum into the angular distribution of scattered light NSTX 50 th Annual Meeting of the Division of Plasma Physics November 17 21, 2008 4
The NSTX collective scattering system measures fluctuations up to k ρ e ª 0.6 280 GHz collective scattering system Five detection channels k spectrum for up to five discrete k k^ρ e d 0.6 and k^ d 20 cm -1 ω spectrum from time-domain sampling 7.5 MS/s f 3.25 MHz Heterodyne detection Tangential scattering Beams nearly on equatorial midplane Sensitive to radial fluctuations Toroidal curvature enhances spatial localization along probe beam, ΔL ~ 10 cm Radial localization, ΔR ~ ±2.5 cm Steerable optics Scattering volume can be positioned throughout the outer half-plasma NSTX 50 th Annual Meeting of the Division of Plasma Physics November 17 21, 2008 5
Steerable optics enable good radial coverage; toroidal curvature enhances spatial localization Large toroidal curvature imposes an instrument selectivity function that constricts the scattering volume within the overlap volume along the probe beam. Mazzucato, PoP, 2003 Mazzucato, PPCF, 2006 NSTX 50 th Annual Meeting of the Division of Plasma Physics November 17 21, 2008 6
Scattering system hardware BWO source ~100 mw at 280 GHz Overmoded, corrugated waveguide low-loss transmission Probe & receiving beams quasi-optically coupled with 5 cm dia. waist Heterodyne receiver five channels two mixing stages quadrature detection with 7.5 MHz bandwidth reference signal from BWO D. R. Smith et al, in press, RSI NSTX 50 th Annual Meeting of the Division of Plasma Physics November 17 21, 2008 7
Toroidal rotation from NBI produces a Doppler shift in fluctuation spectra toward the ion drift direction 3.5 kg, 700 ka, 4 MW NBI, R=133 cm, r/a 0.55 Spurious reflections of the probe beam produce the ubiquitous interferometric signal at 0 Hz. NSTX 50 th Annual Meeting of the Division of Plasma Physics November 17 21, 2008 8
Enhanced fluctuations observed in core region of high-te L-mode plasma 5.5 kg, 600 ka, 1.2 MW HHFW, R=120 cm, r/a 0.28 NSTX 50 th Annual Meeting of the Division of Plasma Physics November 17 21, 2008 9
Enhanced fluctuations occur when Te exceeds the ETG critical gradient Mazzucato et al, PRL, 2008 NSTX 50 th Annual Meeting of the Division of Plasma Physics November 17 21, 2008 10
Enhanced fluctuations observed in core region of NBI-heated H-mode plasma 4.5 kg, 700 ka, 4 MW NBI, R=113 cm, r/a 0.15 NSTX 50 th Annual Meeting of the Division of Plasma Physics November 17 21, 2008 11
Enhanced fluctuations generally occur when Te exceeds the ETG critical gradient NSTX 50 th Annual Meeting of the Division of Plasma Physics November 17 21, 2008 12
Enhanced fluctuations observed at mid-radius in NBI-heated H-mode plasma 4.5 kg, 700 ka, 4 MW NBI, R=133 cm, r/a 0.55 NSTX 50 th Annual Meeting of the Division of Plasma Physics November 17 21, 2008 13
Near ETG marginal stability, fluctuation amplitudes decrease when the E B shear rate exceeds the ETG growth rate D. R. Smith et al, to be submitted to PRL NSTX 50 th Annual Meeting of the Division of Plasma Physics November 17 21, 2008 14
E B shear rate is larger at higher B T, yet enhanced fluctuations are still observed 5.5 kg, 700 ka, 4 MW NBI, R=133 cm, r/a 0.55 NSTX 50 th Annual Meeting of the Division of Plasma Physics November 17 21, 2008 15
Near ETG marginal stability, fluctuation amplitudes decrease when the ETG growth rate drops below the E B shear rate NSTX 50 th Annual Meeting of the Division of Plasma Physics November 17 21, 2008 16
Fluctuation amplitudes decrease at higher B T with similar E B shear rates, ETG growth rates, and Te NSTX 50 th Annual Meeting of the Division of Plasma Physics November 17 21, 2008 17
In H-mode, k r -spectrum is steeper near core compared to mid-radius NSTX 50 th Annual Meeting of the Division of Plasma Physics November 17 21, 2008 18
Measured k r -spectrum in L-mode plasma is steeper than k r -spectrum from GTS simulation 5.5 kg, 600 ka, 2 MW HHFW, R=119 cm, r/a 0.32 Global NL GTS simulation is electrostatic with adiabatic ions and actual mass ratio NSTX 50 th Annual Meeting of the Division of Plasma Physics November 17 21, 2008 19
Summary The NSTX collective scattering system is a valuable tool for investigating ETG turbulence Enhanced fluctuations coincide with Te exceeding the ETG critical gradient Fluctuation amplitudes decrease when the E B shear rate exceeds the ETG growth rate Fluctuations amplitudes decease at higher B T In H-mode, k r -spectrum is steeper near core compared to mid-radius Comparisons between measured fluctuations and global nonlinear GTS simulations have begun NSTX 50 th Annual Meeting of the Division of Plasma Physics November 17 21, 2008 20